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The Physics of the Sodium Laser Guide Star: Predicting and Enhancing the Photon Returns

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The Physics of the Sodium Laser Guide Star: Predicting and Enhancing the Photon Returns THE PHYSICS OF THE SODIUM LASER GUIDE STAR: PREDICTING AND ENHANCING THE PHOTON RETURNS Edward Kibblewhite University of Chicago ABSTRACT Not all lasers give the same photon return/watt and it is this parameter, rather than the raw power generated by the laser, that is the more important figure of merit. In this paper we outline the physical processes involved in calculating this photon return from different types of laser, starting off with the single frequency CW laser developed at the SOR facility. Methods of increasing the return are then discussed and recent experimental results from chirping experiments at Palomar Observatory presented. 1. INCREASING THE COLUMN DENSITY OF SODIUM ATOMS IN THE MESOSPHERE About 100 tons of meteorite burn up in the upper atmosphere every day, producing of about 100 kg of sodium metal [1]. The metal is removed by various complex physical and chemical processes, which ionize the atoms at high altitudes and lock the sodium atoms either into chemicals or on the surface of sub-micron sized “smoke” at altitudes below 85 km [1]. The total mass of sodium available in the entire mesosphere for generating a guide star is about 500 kg, implying a lifetime of about 5 days, with significant annual and diurnal variation. Greatly enhanced short-lived sodium abundances , so-called “sporadic” sodium , occur on shorter time scales which can increase the abundance by over a factor of ten for periods of minutes to hours [2]. Typical column densities are between 2 and 7 x 1013 atoms/m2 with peak densities sometimes exceeded 20 x 1013 atoms/m2 [2]. It is remarkable that so little sodium metal can backscatter even a few per cent of the radiation from a laser beam and it is conceivable that a few tens of kg of sodium metal, suitability dispersed, could greatly increase the brightness of the LGS locally but for periods of hours. Should such a technology prove feasible, the use of potassium metal, which occurs at a favorable wavelength for laser technology and could allow two-frequency LGS AO, might be even more effective. Such a strategy would be expensive but might of value for important transient targets. In the meantime the only way to increase the return is to build either more powerful lasers or improve the efficiency of producing photons from the sodium atoms. 2. OPTICAL PUMPING IN THE SODIUM ATOM It is well known [5] that, for the D2 line used to produce laser guide stars, the sodium atom has two ground levels, an upper F=2 state and a lower F = 1 state, with 5/8 of the atoms being in the F=2 state under conditions of thermal equilibrium. The upper F levels is split into 4 hyperfine sublevels each separted by some tens of MHz. All levels are additionally divided into different M levels, which have the same energy but different cross-sections to the radiation field. A simplified energy diagram of the atom is shown in figure 1. If right handed circularly polarized photon of the appropriate frequency excites a sodium atom in the (2,M) ground state to the upper (3,M+1) level, it can decay to the (2,M), (2,M+1) or (2,M+2) ground level. If this is repeated and in the absence of other effects, the atom will then be optical pumped into a stable transition between the (2,2) and (3,3) state after a small number of cycles. Since this transition has the highest cross-section to the radiation field and highest backscattering efficency to ground, this optical pumping mechanism is very useful in increasing the photo return. We should note that the enhanced return is not only because of the enhanced backscatter return for this transition (a factor of 1.5 compared to isotropic scattering) but also because the cross-section is a factor of about 2 higher than the cross-section averaged over all M levels. We expect an increase in photon return of a factor of about 3 and this has been observed at MIT/Lincoln Labs with a suitably tailored laser spectral format and a well resolved spot [3]. However, we can also see from figure 1 that the photon return can be significantly reduced by depopulation of the F=2 ground state by another optical pumping process as follows. If the sodium atom is moving in slightly different direction, the energy diagram may favor transitions from the F =2 ground state to either the F=1 or F=2 upper state. For these excited atoms there is now a choice of ground state; an atom starting in the same ground (2,0) level may get excited to the upper (2,1) or even the (1,1) level and on decay may go either to the original F=2 ground state or the F=1 ground state. Because the energy separation between the two ground states (1.77 GHz) is substantially larger than the Doppler linewidth (500MHz HWHM), an atom pumped to the F=1 state will have minimal photon interaction with a single frequency laser tuned to pump atoms in the F=2 ground level and the photon return will be correspondingly reduced. There are thus two competing optical pumping processes at work, one pumping the atom to a favorable and stable (2,2) to (3,3) transition and one pumping atoms depopulating the upper ground state so that they no longer interact with a single frequency laser beam. Figure 1: Simplified energy diagram of the Sodium D2 transitions. The two ground states are separated by 1.771 GHz. 3. INTERACTION OF THE SODIUM ATOM WITH ITS ENVIRONMENT Other physical processes are also important and the environment of the mesosphere plays a critical role in the laser-atomic interactions. Firstly, the natural linewidth of the D2 line is only 10 MHz FWHM, which is much narrower than the Doppler width of 1 GHz for atoms at temperature of 200oK. This is shown in figure 2 F=2 -> F=3 Velocity distribution F=2 -> F=2 F=2 -> F=1 Figure 2: Doppler line of sight velocity distribution of sodium atoms in the mesosphere compared to the natural line width of the sodium D2 line Let us assume that that a single frequency CW laser is tuned to the zero velocity frequency of the F=2 to F=3 transition of the D2 line. Because the natural line-width is so narrow, only a few per cent of the atoms, moving in a direction approximately orthogonal to the laser beam, have a strong interaction with the radiation field. An atom with a zero line of sight velocity will absorb and spontaneously reemit one photon every 170 nsec for a laser beam intensity of 10 watts/m2 and will continue to reemit photons until it collides with an air molecule. It will then usually move in different direction and only minimally interact with the radiation field, until it finds itself again with another near-zero line of sight velocity after yet another collision. Sodium atoms in the mesosphere therefore emit photons in bursts when excited by a single frequency laser. A sodium atom that has made either the transition to the upper F=1 or F=2 state has about an even chance of ending up in the lower F=1 ground level. Transitions to these upper F=1 and F=2 levels produce little extra light but enable substantial loss of atoms in the F=2 ground state to occur. It is important to realize that these transitions effect the total population of sodium atoms because even atoms moving in a direction hundreds of MHz from the laser line still have a small chance of interaction with the radiation field and, over a collision lifetime (100 µsec), can get pumped to the lower level - a cycle time of 50 µs is all that may be needed for a velocity class to be depopulated. This is shown in figure 3, which presents the number of atoms in the upper level as a function of Doppler velocity after a collision lifetime of 100 µsec. The laser has an intensity a 200 w/m2, which typical for next generation LGS AO facilities. If there were no depopulation pumping, the curve would follow the conventional Doppler Gaussian curve, with a FWHM of about 1 GHz. Because of depopulation, a single frequency laser depopulates about 40% of the atoms in the upper ground state in100 µseconds (figure 3a). The situation is much worse for multi-line lasers, such as are used at the Gemini Observatory, essentially all the atoms being pumped to the lower level after 100 µseconds (figure 3b) 14 25 (a) 12 F=2 population with no (b) depopulation 10 20 F=2 population 8 15 with depopulation 6 10 4 5 2 - 1000 - 500 500 1000 - 1000 - 500 500 1000 Line of sight velocity in MHz Line of sight velocity in MHz Fig ure 3: Po pulation remainin g in the F=2 grou nd state after a 100 µsecond collision lifetime for a laser intensity 2 of 2 00 w/m . These figures include the effects of radiation pressure, Zenith pointing, 0.5 gauss magnetic field at an angle of 300 to the laser beam. (a) is for a single frequency CW laser (b) is for a laser with lines spaced 98 MHz apart under a Gaussian envelop of 800 MHz FWHM. Spin Exchange Collisions of sodium atoms with nitrogen molecules cannot bring the ground states back into thermal equilibrium. If this was the only mechanism for rethermalization we would be dependent on the flow of new atoms into the laser beam either by diffusion or mesospheric wind [5], both of which have typical time scales of a few milliseconds.
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